HSC 1150

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0.25 UTI
0.0
CN
1.0
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.6 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1150 is a sparse, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 51.932 55.34 0.564 1.067 -0.516 -47.073
Hunt & Reffert 2024 51.929 55.343 0.568 1.083 -0.475 –
Cavallo et al. 2024 51.978 55.291 0.573 – – –
Hunt & Reffert 2023 51.929 55.343 0.568 1.083 -0.475 –

💡 Note: The UCC values are estimated from its identified members.

Reference Year Dist [kpc] Av [mag] DAv [mag] Age [Myr] [Fe/H] [dex] Mass [Msun] Bfr BSS
Hunt & Reffert 2024 – – – – – 138* – –
Cavallo et al. 2024 1.91 2.95 – 35 0.240 – – –
Hunt & Reffert 2023 1.68 3.02 0.93 36 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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